Left: HARPS-N CCFs obtained on four consecutive nights, showing a wide main component at about −80 km s^-1, and more subtle CCFs around 100 km s^-1. Right: best-fit orbital solution for the three components of the system (black: A; blue: Ba; red: Bb), and the residuals of the fit shifted for clarity (points near dashed line). These are ~1.6 km s^-1 for the A component and ~11 km s^-1 for each of the components of binary 1.